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Mazzitelli, I. |
Volume |
Paper Title |
Page Number |
Authors |
40 |
Test of a new theory for stellar convection using helioseismology |
63 |
Paterno, L.; Ventura, R.; Canuto, V. M.; Mazzitelli, I. |
40 |
Main sequence structures including the overdiabatic CM convection model |
457 |
Mazzitelli, I.; D'Antona, F. |
78 |
A Large Astrophysical Database of Stellar Evolutionary Tracks: First Application to Globular Clusters Ages |
411 |
Mazzitelli, I.; Caloi, V.; D'Antona, F. |
134 |
A Role for Superadiabatic Convection in Low Mass Structures? |
442 |
D'Antona, F.; Mazzitelli, I. |
138 |
Selfconsistent model for turbulent convection: helioseismology, ages of globular clusters, and white dwarfs blue edge |
123 |
Goldman, I.; Canuto, V. M.; Mazzitelli, I. |
173 |
A Ready to Use Post-MLT Recipe for General Stellar Modelling and Evolution |
77 |
Mazzitelli, I. |
173 |
Coupling Between Diffusive Mixing and Nuclear Reactions: Production of Lithium in Massive AGB Stars |
281 |
Mazzitelli, I.; D'Antona, F.; Ventura, P.; Zeppieri, A. |
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